PTYS 214 Spring Announcements. Midterm #4 one week from Tuesday!

Similar documents
PTYS 214 Fall Announcements. Materials from last week moved to web page. Midterm #4 next Tuesday!

PTYS 214 Spring Announcements Midterm #4: two weeks from today!

Biodiversity Through Earth History

History of life on Earth Mass Extinctions.

Causes of Extinction

Earth History. What is the Earth s time scale? Geological time Scale. Pre-Cambrian. FOUR Eras

Biodiversity Through Earth History. What does the fossil record tell us about past climates and past events?

Ch. 17 Review. Life in the Cretaceous

Mass Extinctions of the Phanerozoic: The Big Five Total number of families end Ord.

EARTH S HISTORY. What is Geology? logy: science. Geology is the scientific study of the Earth, including its:

5/3/17. Extinction of the Dinosaurs. Extinction of Dinosaurs - Causes. #40 Meteorite Impacts III - Dinosaur Extinction, Future Risk, Mitigation

Where did all the dinosaurs go?

What we ll learn today:!

The History of Life on Earth

LECTURE #25: Mega Disasters - Mass Extinctions, Meteorite Impacts...

The History of the Earth

GO ON. Directions: Use the diagram below to answer question 1.

NATS 101 Section 13: Lecture 32. Paleoclimate

ASTR 380 Mass Extinctions.

IX Life on Earth.

ESA's Rosetta spacecraft What are habitable exoplanets? Is there an Earth 2.0?

Chapter Introduction. Chapter Wrap-Up. Explosion

(continued) Stephen Eikenberry 11 September 2012 AST 2037

Exemplar for Internal Achievement Standard. Earth and Space Science Level 2

Please take out your fill-in notes again, and we will continue learning about extinct creatures.

A brief history of the Earth!

Chapter 9 Remnants of Rock and Ice. Asteroids, Comets, and Pluto

17-1 The Fossil Record Slide 2 of 40

Chapter 19: Meteorites, Asteroids, and Comets

What is the K/T boundary?

Earth & Earthlike Planets. David Spergel

Phys 214. Planets and Life

The History of the Earth

Terrestrial Planetary Atmospheres

Activity 1-2: Origin of the Earth

sparked by just the right combination of physical events & chemical processes Life s Origin & Early Evolution (Ch. 20)

GLY August, Ms. Nelda Breedt. Fragment of extra-terrestrial material that strikes the surface of the Earth.

Outline. Origin and History of Life

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

Outline 9: Origin of the Earth: solids, liquids, and gases

0 questions at random and keep in order

Impacts from Above. Mass Extinctions: Death and Destruction

Chapter 12. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 34: Asteroids and Comets [4/13/07] Announcements. Near-Earth Objects

Asteroids: Introduction

5 Time Marches On. TAKE A LOOK 1. Identify What kinds of organisms formed the fossils in the picture?

HOW GEOGRAPHY AND GEOLOGY AFFECT BIOLOGICAL DIVERSITY

Two significant figures are enough! You can round your calculations to 2 significant figures. Hopefully this will prevent some of the sloppy

Lecture #19. Evolution of Humans. Next Week: Habitability! Chpt 7

17-1 The Fossil Record Slide 1 of 40

GEOL 02: Historical Geology Lab 12: The Mesozoic Dies

FOLLOWING THE TRAIL OF EVIDENCE

Phanerozoic Diversity and Mass Extinctions

Pluto s orbit is tilted and significantly elliptical. Neptune orbits three times during the time Pluto orbits twice resonance prevents a collision.

PTYS 214 Spring Announcements. Get exam from Kyle!

Phanerozoic (last 0.54 by) Tectonics Climate Life

Cycles in the Phanerozoic

Chapter 11. The Archean Era of Precambrian Time

Lecture 20. Origin of the atmosphere (Chap. 10) The carbon cycle and long-term climate (Chap. 8 of the textbook: p )

Geological Time Scale UG Hons.1 st Year) DR. CHANDAN SURABHI DAS ASST. PROF. IN GEOGRAPHY BARASAT GOVT. COLLEGE

The Phanerozoic Eon. 542 mya Present. Divided into 3 Eras The Paleozoic, Mesozoic, and Cenozoic Eras

Finding Impact Craters with Landsat

Geosphere Final Exam Study Guide

Homework #3 is due Friday at 11:50am! Nighttime observing has 10 more nights. Check the webpage. 1 st exam is October 10 th 2 weeks from Friday.

Outline. Atoms in the Solar System. Atoms in the Earth. Back to Atoms for fun The Earth as a Planet. Homework #3 is due Friday at 11:50am!

Chapter 14: The Changing Climate

STAAR Science Tutorial 48 TEK 8.11C: Effects of Environmental Change

SIO15 Midterm 1, Monday Oct. 30, 2017 TEST VARIATION: 2

How do we learn about ancient life? Fossil- a trace or imprint of a living thing that is preserved by geological processes.

Station Look at the fossil labeled # 16. Identify each of the following: a. Kingdom b. Phylum c. Class d. Genus

Structure of the Earth EARTH ( ) - need a solid, will not go through a liquid

What is Earth Science? Earth science is the branch of science dealing with the constitution of the earth and its atmosphere.

4 Changes in Climate. TAKE A LOOK 2. Explain Why is more land exposed during glacial periods than at other times?

Chapter 12 Remnants of Rock and Ice. Asteroid Facts. NEAR Spacecraft: Asteroid Eros

The Cycling of Matter. Day 1

Mass Extinctions &Their Consequences

Griffith Observatory Samuel Oschin Planetarium. Griffith Observatory Samuel Oschin Planetarium. Griffith Observatory Samuel Oschin Planetarium

Chapter 12 - Long term climate regulation. Chapter 10-11* -Brief History of the Atmosphere. What is p really about? New and improved!

Chapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

Eras of Earth's History Lesson 6

Name Date Class. Directions: Use the diagram below to answer question Florida Progress Monitoring and Benchmark Assessments

Teacher Background. Impact! Down to Earth KS 3&4

Earth s History. The principle of states that geologic processes that happened in the past can be explained by current geologic processes.

Earth as Planet. Earth s s Magnetic Field. The Earth s s Crust. Earth s s Interior

Biology. Slide 1 of 40. End Show. Copyright Pearson Prentice Hall

TAKE HOME EXAM 8R - Geology

The Official CA State Science Education Standards for Earth Science K 8

Page 143: Geologic Time

Prentice Hall: Science Explorer, 16 Book Series 2005 Correlated to: Alabama Science Standards for Earth and Space Science Core (Grade 6)

The Good Earth: Introduction to Earth Science 3rd Edition Test Bank Chapter 03 - Near-Earth Objects

Impact Events in Earth History: The Cretaceous-Paleogene Boundary Ejecta Layer and its Source Crater at Chicxulub

The Cosmic Perspective Seventh Edition. Asteroids, Comets, and Dwarf Planets: Their Natures, Orbits, and Impacts. Chapter 12 Review Clickers

Rocks and the Rock Cycle. Banded Iron Formation

Question #1: What are some ways that you think the climate may have changed in the area where you live over the past million years?

Climate Regulation. - What stabilizes the climate - Greenhouse effect

The Sun and Planets Lecture Notes 6.

Earth s Formation: 4.6 Billion Years ago

1 Earth s Oceans. TAKE A LOOK 2. Identify What are the five main oceans?

The Terrestrial Planets

Chapter 2 Geography. Getting to know Earth

12.3 Pluto: Lone Dog No More

Transcription:

PTYS 214 Spring 2018 Announcements Midterm #4 one week from Tuesday! 1

Previously Atmospheric O Respiration UV protection; O2, O3 O sources / sinks Evidence for early O history BIFs Sulfur MIF Forest fires etc... O / life history > 2.5 Ga (Archean): >.5 Ga (Proterozoic): present (Phanerozoic): 1 ppm few % 15--35% single-celled primitive multi-celled macroscopic life Logistic growth / Mass extinctions 2

Taxonomy Species: Homo Sapiens (all people) Genus: Homo (humans and close relatives) Family: Hominidae ( great apes : humans, chimpanzees, gorillas, orangutans) Order: Primates (all apes and monkeys) Class: Mammalia (mammary and sweat glands) Phylum(division): Chordates (vertebrates) Kingdom: Animalia (moving consumers) Domain: Eukarya (complex cells) 3

Mass Extinctions Sharp decrease in the number of species in a relatively short period of time Rapid event - 10,000 to 100,000 years A significant part of all life on Earth became extinct (use of genera or families is more reliable than species; for example extinction of 18% of all families corresponds to about 40% of all genera and 70% of all species) Extinct life forms from various phyla, lived in different habitats, spread out over the whole world 4

Mass Extinctions All genera Well- defined genera Trend line Big Five mass extinctions Other mass extinctions >15% of animal families died or > 40% of animal genera died The Big Five : 1) Cretaceous/Paleogene (K/Pg or K/T): ~65 Myr ago 2) Triassic-Jurassic: ~205 Myr ago 3) Permian-Triassic: ~251 Myr ago 4) Devonian-Carboniferous: ~365 Myr ago 5) Ordovician-Silurian: ~445 Myr ago 5

Studying Extinctions The older the fossil record gets, the more difficult it is to read it (and the less samples that are available)! Use indirect evidence as well, like isotopic changes (for example, 13C) After a mass extinction fauna and flora are dominated by opportunistic species ('weeds', 'pests ) After a mass extinction species experience rapid reproduction, diversification 6

Cretaceous/Paleogene (K/Pg) Extinction (Formerly Cretaceous / Tertiary (K/T) 65 million years ago at least 75% of animal species (17% of all families) went extinct in a very short interval of geologic time PALEOGENE AFFECTED LAND AS WELL AS SEA LIFE Many types of fossil disappeared fossils found above the boundary are much smaller and less abundant than below K/P boundary 7

Geologic K/Pg Boundary Global clay layer up to ~1 cm thick First major stratigraphic boundary identified (early 1800s) shows dramatic change in the types of fossils deposited on either side of this boundary Divides the "Age of Dinosaurs" from the "Age of Mammals Raton Basin, NM, USA 8

The Impact Theory No Dinosaur Tertiary Fossils Clay layer clay layer Dinosaur Cretaceous Fossils Iridium A team led by Walter Alvarez (a geologist) and his father Luis (a Nobel physicist) discovered that the clay layer contains an anomalous high concentration of iridium Alvarez et al (1980) Extraterrestrial cause for the Cretaceous-Tertiary extinction. Science 208, 1095-1108 9

The Iridium Anomaly Siderophile (iron-loving) element - dissolves in molten iron Abundant in meteorites Chondrite What about the Earth? Ir is depleted in the Earth s mantle and Earth s crust; why? Iridium is more abundant in meteorites, i.e., asteroids, than in Earth s surface rocks, so the Alvarez team proposed that a large asteroid impacted Earth at that time One small problem Where is the crater? 10

Over the years additional evidence accumulated Impact-indicators were found worldwide: - Iridium - Stishovite/coesite (Shocked Quartz) - Microtektites (molten spherules) 11

0.32 mm quartz grain Shocked Quartz Under intense pressure (but limited temperature), the crystalline structure of quartz is deformed along planes inside the crystal (planar deformation features) 12

Spherule layer (microtektites) K/Pg Spherules Archean Spherules Microscopic glassy particles formed from molten rock ejected from the impact craters Smit, J. (1999) Annual Review of Earth and Plan. Sci. 27, p. 83 13

Impact Cratering Like in a large explosion, a lot of energy is used to break, melt, vaporize material Very fast (few seconds to a few minutes) Very high temperatures and pressures Crushing - Melting - Vaporization Trinity test + 3 sec. Comet (D=10 km) 10 km Ocean (4 km) Crust Trinity test + 10 sec.14

Impact Cratering Like in a large explosion, a lot of energy is used to break, melt, vaporize material Very fast (few seconds to a few minutes) Very high temperatures and pressures Crushing - Melting - Vaporization Trinity test + 3 sec. 10 km Trinity test + 10 sec.15

The Earth has many impact scars Barringer Crater 1200 m (0.75 miles) in diameter, Produced by a 30-40 m object about 49,000 yr ago Manicouagan 100 km in diameter Produced by an asteroid about 5 km in diameter ~ 210 Myr ago 16

Very large impact craters can be seen on the Moon 17

Large impacts are rare! And Earth has plate tectonics! May be difficult to find the K/Pg crater 18

Florida The K/Pg crater The Chicxulub crater in the Yucatán peninsula, Mexico, is widely accepted as the K/Pg impact crater Age: ~65 million years BIG! 195 km Gulf of Mexico Cuba Central America BURIED (1 km of sediments) NASA-JPL Shuttle Radar Topography mission Schrodinger, Moon Galle, Mars Hildebrand et al. (1991) Geology 19, 867-870 19

Consequences of the K/Pg impact Tsunami Hours Waves created by an impact in the ocean Only affects coastal regions After initial devastation, back to normal Important Reminder: Over 70% of the Earth s surface is covered by deep oceans and seas Oceanic impacts are ~3 times more likely than land impacts K/Pg impactor occurred into a shallow sea Not a rare event, more like a typical occurrence 20

Global Consequences of the K/Pg impact Heat Pulse Hours-Days Re-entering ejecta heats up as it goes through the upper atmosphere (friction!) to 1,000K 1,500K Hot ejecta cools down by radiating IR (thermal) energy Surface receives a significant amount of thermal radiation 21

Global Consequences of the K/Pg impact Heat Pulse & Wildfires Hours-Days Ground may have been similar to an oven set to broil for about 20 minutes! Affects land regions, killing above ground animals Not enough to trigger wildfires everywhere on Earth (probably not enough to kill all above ground animals)! Goldin and Melosh, Geology 37, p1135-1138, 2009 22

Global Consequences of the K/Pg impact Climate Perturbation Few Years Cooling from injection of dust and formation of sulfate aerosols (sulfur released by evaporites) in stratosphere Darkness may last for months! Photosynthesis? Not long enough to trigger an ice age! 23

Global Consequences of the K/Pg impact Acid Rain Gases distributed all over the world Sulphur dioxide released into the atmosphere Few Years Acid rain due to rain-out of sulfate aerosols Damage to vegetation? Acidification of oceans? Gases dissolve in rainwater Acid rain kills plant life, pollutes rivers and streams, and erode stonework 24

Global Consequences of the K/Pg impact Greenhouse Effect Decades or Longer Warming from injection of CO2 (released by shocking carbonates) in the atmosphere Mild Effect Temperature increase: droughts floods Melting of glaciers Not enough CO2 injection for a catastrophic effect! 25

K/Pg Mass Extinction Summary 65 million years ago at least 75% of animal species (about 17% of all families) went extinct in a very short interval of geologic time It affected land AND sea life Best working hypothesis: the extinction was triggered by the large impact event that created the Chicxulub structure It is not clear which consequence(s) associated with the impact was the main cause of the extinction possibly, it was a series of effects 26

Other Suggested Causes Climate Change (either warming or cooling) but how intense, and what caused it? Colossal Volcanic Eruptions but they spanned hundreds of kyr before and after! Sea Level Changes causing extinction in oceans and continental interiors? Methane release from methane clathrate deposits how large and how abrupt is the climatic effect? Nearby Supernova No 244Pu found in iridium layer There may have been a combination of causes! 27

What about other extinctions? All genera Well- defined genera Trend line Big Five mass exctintions Other mass extinctions K/Pg extinction No big iridium spikes or other impact indicators associated with other mass extinctions No major mass extinctions associated with other large craters on Earth Many hypotheses, but we don t quite know what triggered most mass extinction events! 28

Where did the K/Pg impactor come from? Asteroids: small bodies that are made of rock or iron - Located in the Asteroid Belt (between Mars and Jupiter) Comets: small bodies made of rock and ice ( dirty snowball ) - Located in the Oort Cloud and in the Kuiper Belt Outer SS Inner SS Jupiter 29

You Bet Your Life! 3

Question Why do we see more large craters on the Moon than the Earth? a) More material is hitting the Moon b) The Earth has weather c) The Earth's atmosphere shields it d) The Moon has lower gravity e) The Earth has plate tectonics 31

Answer Why do we see more large craters on the Moon than the Earth? b) The Earth has weather e) The Earth has plate tectonics Why? 32

Question Why is Iridium depleted in the Earth's crust? a) It oxidizes when exposed to the atmosphere b) It dissolves in iron c) It is precipitated on the ocean floor d) It is depleted in asteroids e) It dissolves in silicate rocks 33

Answer Why is Iridium depleted in the Earth's crust? b) It dissolves in iron Why? 34

Question Which of the following are evidence that the K/Pg boundary is associated with an impact? a) An Ir anomaly b) Shocked quartz c) A mass extinction d) Microtectites e) Major volcanic eruptions 35

Answer Which of the following are evidence that the K/Pg boundary is associated with an impact? a) An Ir anomaly b) Shocked quartz d) Microtectites Why? 36

Question Which of the following are evidence that the Chicxulub crater is associated with the K/Pg extinction? a) Its age b) Shocked quartz c) Its size d) Microtectites e) Its shape 37

Answer Which of the following are evidence that the Chicxulub crater is associated with the K/Pg extinction? a) Its age c) Its size Why? 38

Homework Homework #16 available shortly on the web site 39

https://www.youtube.com/watch?v=cdhh3df bico https://www.youtube.com/watch?v=fnfzfwl M72c